It is quite obvious that an azimuthal mount causes field rotation,
when not used on the North- or the South-pole. For real long
exposures (i.e. minutes to hours) this is utterly devastating for
every image taken.
Here the abilities and power of CCDs are coming
into play. With exposure times of a couple of seconds, field rotation
does not play any role for the single frame. As long as the CCD
amplifier ensures that the charge in a single pixel is high enough to
result in a signal greater than the detection threshold we can
integrate over several different frames. Now field rotation will
return when not properly taken care of .
IRIS
however is capable to compensate for rotation between individual
frames during alignment. Lets see what is to be done, on a step by
step basis, assuming the raw fits series (after conversion) is called
r#.fits (for red), g#.fits (for green) and b#.fits (for blue).
Furthermore assume that the data set contains 50 frames.
Get a “Display commands window” first.
If not using IRIS in the first place you most likely have to convert your AVI-file into a plurality of FITS-files. When going for color, every frame will be present in a red, a green and a blue channel in separate FITS-files. That means, that you will have to perform all following steps on a respective color files individually. Conversion done by: [click: File -> AVI conversion... ].
Now you will have to select two suitable objects (stars) by
marking.
For this you have to get one frame into the main
window, preferably the first of a series: [type: load r1].
Now
mark two medium-bright stars which are not too close to each other:
[click: Analysis -> Select Objects => with the funny mouse
pointer click on two medium-bright stars].
If everything went fine so far, you will be ready for
registering the frames yet: [type: rregister r rr 100 50].
A new
file-set with the name rr will be created. Forget about the third
parameter for the moment, you will learn to use it with some
practice.
With the time it will become clearer which registration
objects will give better results and what combination will not be so
good.
Stacking registered frames, nothing easier than this: [type: add2 rr 50].
Now you certainly would like to save the result: [type: save red].
Do the same with the other two colors...
To combine the three images you could do all sorts of tricks
with IRIS. A simple first glance could be: [type: trichro red green
blue].
Save your result by: [type: savebmp myimage].
Have a look at an example analysis done on M52 data. Both results came from the same data set, analysed in different ways.
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M52, ETX-70, analysed with K3CCDTools, dark frame subtracted |
M52, ETX-70, analysed as described above, no dark frame subtraction |
last modified 10.01.05